A comparison of polycyclic aromatic hydrocarbon emission in low- and high-metallicity environments suggests that the growth of these molecules is inhibited in low-metallicity environments, resulting in lower emission.

The supernova remnant SN 1006 shows a high degree of X-ray polarization, and the degree of polarization varies with location; the polarization is lower where the shell is thought to interact with an interstellar cloud.

Using the interferometric capabilities of the Canadian Hydrogen Intensity Mapping Experiment, astronomers have localized a seemingly non-repeating fast radio burst to a galaxy just 130 million light-years away.

Researchers describe the current state of knowledge regarding Europa’s plumes and the Europa Clipper search strategy, which involves an initial global search that will be used to guide later observations.

Near-infrared spectra and images have revealed that the central source of the H II region is an early B-type star, and that stellar feedback is actively shaping the environment of the star-forming region.

Using a high-resolution simulation, a researcher has reproduced the Sun’s near-surface shear layer for the first time, leading to improved understanding of how the layer is constructed.